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formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory)
From: "Jonathan Thornburg [remove -animal to reply]"
Subject: formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory) Newsgroups: sci.astro.research References: [[I've changed the subject line, as this discussion no longer has much of anything to do with Kepler's results or planetary formation theory]] Robert L. Oldershaw wrote: In the Jan. 14th issue of Nature is a paper that claims to resolve a serious problem that has plagued the CDM cosmology for a long time. [[...]] For the benefit of others, the paper in question is this one: F. Governato, C. Brook, L. Mayer, A. Brooks, G. Rhee, J. Wadsley, P. Jonsson, B. Willman, G. Stinson, T. Quinn & P. Madau "Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows" Abstract: For almost two decades the properties of `dwarf' galaxies have challenged the cold dark matter (CDM) model of galaxy formation1. Most observed dwarf galaxies consist of a rotating stellar disk2 embedded in a massive dark-matter halo with a near-constant-density core3. Models based on the dominance of CDM, however, invariably form galaxies with dense spheroidal stellar bulges and steep central dark-matter profiles4, 5, 6, because low-angular-momentum baryons and dark matter sink to the centres of galaxies through accretion and repeated mergers7. Processes that decrease the central density of CDM halos8 have been identified, but have not yet reconciled theory with observations of present-day dwarfs. This failure is potentially catastrophic for the CDM model, possibly requiring a different dark-matter particle candidate9. Here we report hydrodynamical simulations (in a framework10 assuming the presence of CDM and a cosmological constant) in which the inhomogeneous interstellar medium is resolved. Strong outflows from supernovae remove low-angular-momentum gas, which inhibits the formation of bulges and decreases the dark-matter density to less than half of what it would otherwise be within the central kiloparsec. The analogues of dwarf galaxies-bulgeless and with shallow central dark-matter profiles-arise naturally in these simulations. Nature volume 463, number 7278, pages 203-206 (14 Jan 2010) http://www.nature.com/nature/journal...ture08640.html doi:10.1038/nature08640 preprint (open-access!) at http://arxiv.org/abs/0911.2237 Nature also has an "Editor's summary" and a "News and Views" article about this work, Marla Geha "Galaxy formation: Gone with the wind?" Nature volume 463, number 7278, pages 167-168 (14 Jan 2010) http://www.nature.com/nature/journal...l/463167a.html doi:10.1038/463167a So now international teams of theorists using "millions of hours on supercomputers" have run SIMULATIONS that reproduce the desired phenomenon. Just so! Break out the champagne! Mission Accomplished! But does anyone else see some reasons for very serious misgivings here? (1) The "correct" answer was assumed to be known from the start. (2) Theorists were not going to give up until they got the "right" answer. I think there may be some misunderstanding here of the role that computers and computer simulations play in theoretical astrophysics. The usual way things get done is this: 1. Someone suggests a physical model (which usually has a bunch of parameters). This might be based purely on speculation, and/or it might be based on analysis of past observatious. In fact, it might be the same as some other model which is already well-known, but this time it's elaborated a bit more. 2. Are people able to solve the model's equations analytically? 2a: Yes -- Goto step 3 to explore the analytical solution 2b: No -- (i) Computational people figure out how to solve the equations numerically (or, if this has already been done, how to solve them more efficiently, accurately, and/or robustly than has been done in the past). If this is a lot of work, write a paper on just this and submit it to arxiv and a journal. (ii) Goto step 3 to explore the numerical solution. 3. Try varying the model parameters to see if we can get reasonable agreement between the model equations' solution (either analytical or numerical) and past observations (if there are any). 4. Try varying the model parameters some more to see if any interesting predictions can be made about what future observations might show. 5. Write papers on steps 3 and 4 & submit them to arxiv and journals. (Papers on step 4 also serve as hints to our observational colleagues that they might try making said observations.) Notice that very little of this process (only steps 2a vs 2b) depends on whether computers are used. As Forman Acton has famously said (in his classic (though now rather dated) book "Numerical Methods that Work"), "the purpose of computing is insight, not numbers". Notice also that the process is actually very similar regardless of whether the observations predate or postdate the theoretical calculation. (3) Using computers and many adustable parameters you can get whatever you want. I'm sorry, but that's simply not true. It may be that for *some* physical systems (the models for which might have analytical solutions, or they might not) with many adjustable parameters, you can get a wide range of qualitative behavior. But that's certainly not the case for all physical systems, or even for all physical systems whose equations need a computer to solve. A case in point: Consider a bound binary black hole system in an otherwise empty asymptotically flat spacetime, with dynamics given by general relativity. This system has around 15 parameters, and simulating its outcome takes a lot of computer time (on the order of 10,000 - 100,000 CPU-hours for a medium-resolution simulation). But despite that, (I hereby assert) *no* combination of those parameters will result in the binary becoming unbound. Indeed, *no* combination of those parameters will result in any other final end state than (the two black holes merging to form) a single black hole. (2) Theorists were not going to give up until they got the "right" answer. What the paper in question actually says is that (a) Here's a well-known problem (a bunch of observations which weren't well explained by past theoretical predictions). (b) Here's a particular theoretical model (which the authors argue is better than past models, in that it more accurately approximates what we believe to be the underlying physics than past models did). (c) Here are some (numerical) calculations of that model's outcomes for certain (given) sets of parameters which (the authors assert) are plausible. (d) The calculated outcomes agree pretty well with past observations. Could you be more specific about which of (a), (b), (c), and/or (d) in this paper you consider to be not "right"? Or, if you don't find fault with any of (a), (b), (c), or (d) in this paper, could you explain more clearly just why it is that we should disbelieve the author's conclusions? Do you have any specific evidence that "you can get whatever you want" by adjusting the paremeters in the authors' model? Is there some other reason why we should distrust their model? ciao, -- -- "Jonathan Thornburg [remove -animal to reply]" Dept of Astronomy, Indiana University, Bloomington, Indiana, USA "Washing one's hands of the conflict between the powerful and the powerless means to side with the powerful, not to be neutral." -- quote by Freire / poster by Oxfam |
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formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory)
On Jan 15, 3:30*pm, Jonathan Thornburg
wrote: Do you have any specific evidence that "you can get whatever you want" by adjusting the paremeters in the authors' model? *Is there some other reason why we should distrust their model? Forgive this very brief and partial [] response, but I need to read your post slowly tonight with my happy endings cigar and respond more thoughtfully and fully tomorrow. For now I would just say that we should always maintain a healthy skepticism when dealing with any model-building theory, for the obvious reasons that I have already discussed in the last few days. I repeat my von Neumann paraphrase: "One thinks of Johnny von Neumann's dictum that with 3 variables he could produce an elephant and with 4 variables he could get it to wag its tail. Or something to that effect." He was being humorous, but he was also saying something quite serious. In haste, RLO www.amherst.edu/~rloldershaw |
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formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory)
On Jan 16, 3:52*am, "Robert L. Oldershaw"
wrote: On Jan 15, 3:30*pm, Jonathan Thornburg wrote: Ok, I have had a chance to look over your comments, and I agree this is paper not a "Higgs In Space" pseudoscience paper, but still it raises the definite concerns noted below. (A) Your #1 to #5 list of steps defines the basic strategy of the "Model-Building" approach to physics. I do not believe that this is the best approach to doing physics/science [see Einstein's oeuvre for an elegant and thorough demonstration of how science can be done better]. Sometimes "Model-Building" is the only practical route to go initially and so it can be very useful. HOWEVER, it should be carefully guided and tested by Definitive Predictions at all steps/stages, to the full extent possible. Those who get intoxicated with a model and come to regard it as received wisdom which no longer needs to be challenged empirically, and must be "saved" whatever it takes, are fooling themselves and potentially leading others on a false path. Need I mention the "string theory" fiasco? (B) " (3) Using computers and many adustable parameters you can get whatever you want. I'm sorry, but that's simply not true." I beg to differ, but I will compromise a bit and say one can get "nearly anything" one wants badly enough. (C) This paper is a classic "Save The Phenomenon" paper. That is not to say that it is necessarily a bad paper, or that its results are necessarily wrong. But let's be honest about the motivations of this paper. Give it some objective thought and view the situation from the full historical perspective. You will see that this is a classic STP paper. (D) "Or, if you don't find fault with any of (a), (b), (c), or (d) in this paper, could you explain more clearly just why it is that we should disbelieve the author's conclusions?" It could not be put more simply: they are clearly trying to validate a predetermined desiderata. If this does not cause you to have some serious misgivings, then I am worried for science. (E) "Do you have any specific evidence that "you can get whatever you want" by adjusting the paremeters in the authors' model? " von Neumann knew better than either of us; I let him make the case for me. Best, RLO www.amherst.edu/~rloldershaw |
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formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory)
Robert L. Oldershaw schrieb:
Forgive this very brief and partial [] response, but I need to read your post slowly tonight with my happy endings cigar and respond more thoughtfully and fully tomorrow. As this promises to become the "fight" of the fractal cosmology paradigm against the "rest of the world", i urge all proponents to look for a common scientifuc basis and then advance to the controversial issues. Otherwise the thread wil be a long medieval "Hauen und Stechen", where each side claims the victory. This might be pleasing and full of honour for the fighters but boring for the readers. Regards Jurgen [Mod. note: Quoted text deleted. In particular, if the thread turns into an argument about one participant's personal ideas, it may be more appropriate to take it to private e-mail -- mjh] |
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formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory)
In article , "Robert L.
Oldershaw" writes: (A) Your #1 to #5 list of steps defines the basic strategy of the "Model-Building" approach to physics. I do not believe that this is the best approach to doing physics/science [see Einstein's oeuvre for an elegant and thorough demonstration of how science can be done better]. As a reply to this, let me quote you in another thread: because you say so? Is that your version of scientific falsifiation/ verification tests: whether or not something agrees with your assumptions/biases? Really, sir! I'm sorry, but that's simply not true." I beg to differ, but I will compromise a bit and say one can get "nearly anything" one wants badly enough. because you say so? Is that your version of scientific falsifiation/ verification tests: whether or not something agrees with your assumptions/biases? Really, sir! For some adjusted-after-the-fact definition of "nearly". What was that about being able to adjust things until one gets what one wants? It could not be put more simply: they are clearly trying to validate a predetermined desiderata. If this does not cause you to have some serious misgivings, then I am worried for science. You obviously misunderstand science. The "desiderata" are observations. Obviously, if a model doesn't fit observations, it is wrong, or at least incomplete. This is what one expects to find as observations become better and better. So, the model is modified in that it is made more realistic, based on physical assumptions independent of the observations. Then, one checks if the refined model gives a better fit. What's the problem? |
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formation of dwarf galaxies in CDM cosmology
Robert L. Oldershaw wrote:
Sometimes "Model-Building" is the only practical route to go initially and so it can be very useful. Quite true. And sometimes it is the *only* practical route to go -- some systems are simply too complicated for simple "back of the envelope" modelling to get very far. For example, consider operational weather forecasting: There is no known way to produce a 5-to-8-day weather forecast that's significantly more accurate than climatology (i.e. than simply "forecasting" the long-term average conditions for the current location and time-of-year) for most populated parts of the Earth without having a detailed model of the dynamical and thermodynamical state & time-evolution of the Earth's atmosphere. And such a such a model is *way* too complicated to make-predictions-from without computers. [How did weather forecasts get done before computers? The short answer is that forecasts were a lot less accurate back then, indeed, and that 5-to-8-day forecasts with better-than-climatology accuracy didn't exist. See Joseph J. Tribbia and Richard A. Anthes "Scientific Basis of Modern Weather Prediction" Science v.237 (31 July 1987), 493-499. doi: 10.1126/science.237.4814.493 http://www.sciencemag.org/cgi/conten...n/237/4814/493 for more details.] HOWEVER, it should be carefully guided and tested by Definitive Predictions at all steps/stages, to the full extent possible. [[...]] Those who get intoxicated with a model and come to regard it as received wisdom which no longer needs to be challenged empirically, and must be "saved" whatever it takes, are fooling themselves and potentially leading others on a false path. I emphatically agree with both of these statements. -- -- "Jonathan Thornburg [remove -animal to reply]" Dept of Astronomy, Indiana University, Bloomington, Indiana, USA "Most investment bankers' [...] idea of a long-term investment is thirty-six hours" -- Robert Townsend, "Up the Organization" |
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formation of dwarf galaxies in CDM cosmology (was: Kepler's Recent Results in Contradiction to Standard Planet Formation Theory)
In article , "Robert L.
Oldershaw" writes: As I have also mentioned before, theories of principle are the preferred scientific strategy because they can be definitively tested, whereas in model-building one can "cook" the statistics, the reasoning, the assumptions, the data "cuts", the adjustable parameters, etc., etc.,... and therefore empirical testing of model- building results is far less certain. Yes, we get a successively better fit to observations, but do we get a Ptolemaic fit or a Galilean fit? To me there is a huge difference, although some Platonists may not care one way or the other. A counter-example from recent history: there was a HUGE prejudice in favour of the Einstein-de Sitter model of the universe, but now the consensus is that it is ruled out by many lines of evidence. Why isn't there even one serious science who is a good enough cook to still use this model as his hypothesis? |
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